We apply the picket fence treatment to model the effects brought about by spectral lines on the thermal structure of irradiated atmospheres. The lines may be due to pure absorption processes, pure coherent scattering processes, or some combination of absorption and scattering. If the lines arise as a pure absorption process, the surface layers of the atmosphere are cooler, whereas this surface cooling is completely absent if the lines are due to pure coherent isotropic scattering. The lines also lead to a warming of the deeper atmosphere. The warming of the deeper layers is, however, independent of the nature of line formation. Accounting for coherent isotropic scattering in the shortwave and longwave continuum results in anti-greenhouse co...
The methods of constructing a model atmosphere and computing its theoretical spectrum are reviewed, ...
One of the most intriguing outcomes of the young field of exoplanet research is the emergence of hig...
Observational studies of exoplanets are suggestive of a ubiquitous presence of clouds. The current m...
Context. Semi-grey atmospheric models (with one opacity for the visible and one opacity fo...
Context. Semi-grey atmospheric models (with one opacity for the visible and one opacity for the infr...
Context. The recent discovery and characterization of the diversity of the atmospheres of exoplanets...
Context. The recent discovery and characterization of the diversity of the atmospheres of exoplanets...
Context. The recent discovery and characterization of the diversity of the atmospheres of exoplanets...
in preparation Context. The recent discovery and characterization of the diversity of the atmosphere...
An exact model is proposed for a gray, isotropically scattering planetary atmosphere in radiative eq...
Inhomogeneous cloud formation and wavelength-dependent phenomena are expected to shape hot Jupiter a...
We present a comprehensive analytical study of radiative transfer using the method of moments and in...
Aims. We investigate the effects of coherent isotropic continuum scattering on the formation of spec...
Context. The evolution of stars and planets is mostly controlled by the properties of their atmosphe...
The effects of the nongray absorption (i.e., atmospheric opacity varying with wavelength) on the pos...
The methods of constructing a model atmosphere and computing its theoretical spectrum are reviewed, ...
One of the most intriguing outcomes of the young field of exoplanet research is the emergence of hig...
Observational studies of exoplanets are suggestive of a ubiquitous presence of clouds. The current m...
Context. Semi-grey atmospheric models (with one opacity for the visible and one opacity fo...
Context. Semi-grey atmospheric models (with one opacity for the visible and one opacity for the infr...
Context. The recent discovery and characterization of the diversity of the atmospheres of exoplanets...
Context. The recent discovery and characterization of the diversity of the atmospheres of exoplanets...
Context. The recent discovery and characterization of the diversity of the atmospheres of exoplanets...
in preparation Context. The recent discovery and characterization of the diversity of the atmosphere...
An exact model is proposed for a gray, isotropically scattering planetary atmosphere in radiative eq...
Inhomogeneous cloud formation and wavelength-dependent phenomena are expected to shape hot Jupiter a...
We present a comprehensive analytical study of radiative transfer using the method of moments and in...
Aims. We investigate the effects of coherent isotropic continuum scattering on the formation of spec...
Context. The evolution of stars and planets is mostly controlled by the properties of their atmosphe...
The effects of the nongray absorption (i.e., atmospheric opacity varying with wavelength) on the pos...
The methods of constructing a model atmosphere and computing its theoretical spectrum are reviewed, ...
One of the most intriguing outcomes of the young field of exoplanet research is the emergence of hig...
Observational studies of exoplanets are suggestive of a ubiquitous presence of clouds. The current m...